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Connection between UHECR's and supermassive relic particles

dc.contributor.authorLengruber, L. L.
dc.contributor.authorRosenfeld, Rogério [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T14:07:21Z
dc.date.available2014-05-20T14:07:21Z
dc.date.issued2001-04-01
dc.description.abstractOne of the models proposed for the origin of ultra high energy cosmic rays (UHECR's) suggests that these events are the decay products of relic superheavy metastable particles, which we call S particles. These particles can be produced in the reheating period following the inflationary epoch of the early Universe. We study this possibility and obtain constraints on some parameters such as the lifetime and direct couplings of the X-particle to the inflaton field from the requirement that they are responsible for the observed UHECR flux.en
dc.description.affiliationUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.description.affiliationUnespUNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil
dc.format.extent278-281
dc.identifierhttp://dx.doi.org/10.1016/S0920-5632(01)01283-X
dc.identifier.citationNuclear Physics B-proceedings Supplements. Amsterdam: Elsevier B.V., v. 97, p. 278-281, 2001.
dc.identifier.doi10.1016/S0920-5632(01)01283-X
dc.identifier.issn0920-5632
dc.identifier.urihttp://hdl.handle.net/11449/23633
dc.identifier.wosWOS:000168045200059
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofNuclear Physics B: Proceedings Supplements
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.titleConnection between UHECR's and supermassive relic particlesen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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